Mountain Building in Scotland

Size: px
Start display at page:

Download "Mountain Building in Scotland"

Transcription

1 c Science: a level 3 course Mountain Building in Scotland Prepared for the Course Team by Kevin Jones and Stephen Blake Block 3

2 The SXR339 Course Team Chair Stephen Blake Course Manager Jessica Bartlett (Course Manager) Other members of the Course Team Mandy Anton (Graphic Designer) Dave McGarvie (Author) Gerry Bearman (Editor) Steve Best (Graphic Artist) Nigel Harris (Author) Kevin Jones (Consultant Author) Jann Matela (Word Processing) Ian Parkinson (Reader) Val Russell (Consultant Editor) Professor Rob Strachan, Oxford Brookes University (Course Assessor) Andy Sutton (Software Designer) The Course Team gratefully acknowledges the contributions of Andrew Bell and Fiona McGibbon who commented on the proofs of this book. Other contributors to SXR339 are acknowledged in specific credits. Front cover: Gearr Aonach (left) and Aonach Dubh (right) from the Meeting of the Three Waters, Glen Coe. (David W. Wright, Open University) Back cover: The view westwards from Strath Fionan, near Schiehallion, central Perthshire, to Loch Rannoch. (Nigel Harris, Open University) The Open University, Walton Hall, Milton Keynes MK7 6AA. First published Copyright 2003 The Open University. All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, transmitted or utilized in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without either the prior written permission of the publishers or a licence permitting restricted copying issued by the Copyright Licensing Agency Ltd. Details of such licences (for reprographic reproduction) may be obtained from the Copyright Licensing Agency Ltd. of 90 Tottenham Court Road, London W1P 0LP. Edited, designed and typeset by The Open University. Printed in the United Kingdom by Bath Press, Glasgow. ISBN This book forms part of an Open University course, SXR339 Ancient Mountains: Practical Geology in Scotland. Details of this and other Open University courses can be obtained from the Course Reservations and Sales Office, PO Box 724, The Open University, Milton Keynes MK7 6ZS, United Kingdom: tel. (00 44) For availability of this or other course components, contact Open University Worldwide Ltd, Walton Hall, Milton Keynes MK7 6AA, United Kingdom: tel. (00 44) , fax (00 44) , ouwenq@open.ac.uk Alternatively, much useful course information can be obtained from the Open University s website, 1.1

3 1 Introduction Setting the scene Recognizing ancient mountains Orogeny through geological time Geological time: a brief note Disentangling the continents The collage of ancient orogenic belts in the North Atlantic region What caused the Caledonian Orogeny? The tectonic map of Britain and Ireland The scope of this book 14 2 Britain s oldest rocks: remnants of Archaean crust Introduction The Lewisian Complex The nature, age and origin of the gneiss protoliths Deformation and high-grade metamorphism Basement inliers in the Moine Supergroup Summary of Section Orogenies in the Proterozoic Introduction Palaeoproterozoic rifting, sedimentation and magmatism The Palaeoproterozoic Laxfordian Orogeny Assembly of the Lewisian Complex Formation of Proterozoic crust Synthesis: the broader view of Palaeoproterozoic events Mesoproterozoic events Mesoproterozoic rifting: deposition of the Stoer Group The Grenville Orogeny Neoproterozoic events Early Neoproterozoic continental sedimentation: the Sleat and Torridon Groups Early Neoproterozoic marine sedimentation: the Moine Supergroup The Dava and Glen Banchor Successions Extension-related magmatism Evidence for a Neoproterozoic (Knoydartian) Orogeny? Summary of Section Continental break up and opening of the Iapetus Ocean Introduction The Dalradian Supergroup Dalradian sedimentary basins: seeing through metamorphism Primary rock types and terminology Lithostratigraphic subdivisions of the Dalradian Supergroup Dalradian sedimentation and tectonics Dalradian basin evolution Age of the Dalradian Supergroup Cambrian Ordovician shelf sedimentation in north-west Scotland Summary of Section Arc continent collision: the Grampian phase of the Caledonian Orogeny Introduction Ocean closure during the Grampian phase Ophiolites and the evidence for obduction: a Grampian suture zone? 48

4 4 Mountain Building in Scotland Evidence for an ancient magmatic arc Evidence for an ancient subduction zone: the Clew Bay Complex Summary of Section Structural development of the Grampian Highlands Introduction Structure of the Grampian Highlands The deformation sequence Summary of Section Metamorphism in the Grampian Highlands Introduction The metamorphic map of the Dalradian The relative timing of porphyroblast growth and deformation The absolute timing of metamorphic mineral growth The causes of Grampian metamorphism A synthesis of Grampian metamorphism Summary of Section Summary of Section Exhumation of the Grampian mountains Introduction Uplift and cooling history of the Grampian mountains Magmatism during exhumation The record of exhumation in sedimentary basins Synthesis: time constraints on the Grampian phase How high were the Grampian mountains? Summary of Section Sedimentation and tectonics at a mid-ordovician to Silurian active margin Introduction Mid-Ordovician to Silurian sedimentation in the Midland Valley Terrane Ordovician sedimentation Silurian sedimentation Summary of Section Sedimentation and tectonics in the Southern Uplands Terrane Sedimentation The Southern Uplands as an accretionary prism? Summary of Section Interpretation: regional tectonic framework for the Midland Valley and Southern Uplands Introduction What caused a subduction zone reversal? A missing fore-arc basin? Summary of Section Multiple plate collisions and the end of the Iapetus Ocean Introduction Palaeocontinental reconstructions The global view A model for the closure of the Iapetus Ocean Summary of Section

5 Introduction Tectonics of the Northern Highlands Structure and metamorphism of the Northern Highlands Magmatism and the timing of deformation Regional implications Summary of Section Silurian Devonian strike slip displacements on the Laurentian margin Geometry and amount of displacement Time constraints on fault zone displacements Sinistral displacements in the Southern Uplands Summary of Section Collision of Eastern Avalonia with the Laurentian margin The sedimentary record of a far-felt collision Diachronous collision and terrane linkage Sediment dispersal and basin shallowing Where is the Iapetus Suture? Summary of Section Late Silurian to Early Devonian deformation of Eastern Avalonia The cleavage pattern Time constraints on cleavage formation and deformation Summary of Section Granite magmatism and convergence Origin of the Newer Granites Summary of Section Summary of Section Sedimentation at the end of the Caledonian Orogeny Introduction The Old Red Sandstone and the Devonian Period Distribution and stratigraphy of the Late Silurian to Devonian Basins Sedimentation and tectonics in the Midland Valley Structure of the Midland Valley in the Devonian Period Late Silurian Early Devonian sedimentation A Mid-Devonian hiatus Renewed deposition in the Late Devonian Summary of Section Sedimentation and tectonics in the external basins A southward-migrating mountain front A short-lived Mid-Devonian ocean basin? Summary of Section Orogen-scale drainage and sediment dispersal patterns Summary of Section Legacy 113 Acknowledgements 114 Index 115

6 6 Mountain Building in Scotland 1 Introduction 1.1 Setting the scene Some of Britain s most dramatic scenery is to be found in the Scottish Highlands. The sight of mighty Ben Nevis, the desolate plateau of the Cairngorms, or the imposing landscapes of Glen Coe (pictured on the front cover) can unleash the call of the wild in all of us. Although these landforms were largely carved by glacial activity that ended some years ago, the rocks themselves tell of a much older history. The Scottish Highlands, defined as lying north of the Highland Boundary Fault (Figure 1.1), are primarily composed of metamorphosed sedimentary and igneous rocks intruded by somewhat younger igneous bodies and cut by faults. The metamorphic rocks and igneous intrusions exposed at the surface must have formed within the Earth s crust, and this simple fact indicates that the Highlands are merely eroded stumps of a much higher range of ancient mountains. This book is an account of the origin and demise of that ancient mountain range, based on the geological evidence laid before us in rock exposures. For well over a century, geologists have braved the rain, sun and midges to study the Highlands. Indeed, it was nineteenth-century field geologists working in northern Scotland who established several of the fundamental geological principles that are today almost taken for granted. Notable Victorian scientists such as Ben Peach, John Horne, George Barrow, Edward Bailey, Archibald Geikie, Charles Lapworth and Roderick Murchison were among those who made their names by observing and debating the significance of the rocks of the Highlands. For example, Peach and Horne, with others from the Geological Survey, mapped the rocks of north-west Scotland, recognizing an enormous low-angle fault in which ancient metamorphic rocks had been thrust tens of kilometres westwards over younger sedimentary rocks. This fault is now familiar to geologists across the world as the Moine Thrust (Figure 1.1). Working in the south-eastern Highlands around Glen Clova (Figure 1.1), George Barrow founded the concepts of metamorphic zones and index minerals, which are now universally used to map belts of regional metamorphic rocks. Another example, albeit from further south, is James Hutton s recognition, in 1788, of an unconformity at Siccar Point (Figure 1.1), where red sandstones (of Devonian age) had been deposited on upturned older (Silurian) strata. This and similar observations nearby led him to the revelation that sedimentary deposition had been interrupted by significant earth movements and erosion, requiring a truly dynamic Earth and eons of time. Now, in the era of sophisticated geochemical, geochronological and geophysical methods, geologists are still working to make further sense of the region s dramatic geology in terms of plate tectonics and continental drift. So, the prodigious terrestrial displacements, recognized by Geikie to have formed the Moine Thrust, are now attributed to plate-tectonic collisions that happened almost half a billion years ago. To appreciate the classic geology of the Highlands, the basic geological field relationships remain fundamental, so this book has been written with field evidence very much to the fore. In any story, the events that took place and the order in which they did so are critical. In the story of how the Highlands were built (and then eroded), the nature and relative timing of sedimentation, metamorphism, tectonism (folding and faulting), igneous activity and erosion are all revealed by the rocks. The evidence may come from field relationships, such as those that are pictured throughout this book, or from any one of a number of radiometric dating methods requiring high-precision laboratory instrumentation. Among the latter,

7 Introduction 7 post-devonian Devonian sediments and lavas igneous rocks emplaced during Caledonian Orogeny Shetland rocks deformed and metamorphosed during Caledonian Orogeny Ordovician and Silurian sedimentary rocks Precambrian Basement fault H e thrust 100 km b r i s d e NORTH-WEST HIGHLANDS Moine Thrust Orkney Great Glen Fault r O u t e GRAMPIAN HIGHLANDS (or CENTRAL HIGHLANDS) Inverness Aberdeen Stonehaven Strontian Pitlochry Glen Clova MIDLAND VALLEY Glasgow Edinburgh Siccar Point SOUTHERN UPLANDS Highland Boundary Fault Southern Uplands Fault Figure 1.1 The physical geography and geology of Scotland are dominated by the products of mountain-building events, known collectively as the Caledonian Orogeny, that took place during the Palaeozoic. Some important localities in the historical development of the geological sciences (Glen Clova, Siccar Point and Strontian) are shown in italics.

8 8 Mountain Building in Scotland incidentally, is the rubidium strontium method. This relies on the radiogenic isotope of strontium, an element whose name derives from the village of Strontian in Argyllshire (Figure 1.1), where the element was first discovered in the mineral strontianite. 1.2 Recognizing ancient mountains The great modern mountain ranges of the world, such as the Himalaya, have been built over millions of years, and act as natural laboratories where Earth scientists can study the complex interplay of processes that are active during mountain building. The formation of these great mountains ranges, a process called orogeny, is inextricably linked to the forces generated by the collision of lithospheric plates at destructive plate margins. In these collision zones the crust is thickened by deformation, folding and faulting, and/or by the addition of large quantities of magma. A major consequence of tectonic crustal thickening is that rocks that were once at the surface are buried to great depths and undergo substantial modification during deformation and metamorphism (Figure 1.2). Figure 1.2 Highly deformed and metamorphosed igneous rocks from the Borgie inlier, north coast of Scotland. The uplift of deeply buried rocks is achieved either by erosion or by a combination of erosion and tectonic movements such as faulting, and occurs in response to the isostatic readjustment of the overthickened crust this process is called exhumation. Eventually, over millions of years, exhumation reveals the deeper levels, or roots, of the mountain belt. It follows, therefore, that the existence of ancient mountains can be recognized by the identification of zones

9 Introduction 9 of highly deformed and metamorphosed rocks these zones are called orogens or orogenic belts. The study of these ancient mountain roots provides us with a record of the processes that were active in the deep crust during collision. 1.3 Orogeny through geological time Geological time: a brief note Geological time can be divided into Eons, Eras and Periods, with further subdivisions into Epochs and Ages (Figure 1.3). The order of rock units determined from the principles of superposition and faunal succession produces the lithostratigraphic column, which is based simply on the relative ages of rocks, e.g. Llandovery is younger than Ashgill but older than Wenlock. A second aspect of the stratigraphic column relates to the chronostratigraphic dating of rock units, which allows geologists to apply absolute ages to rock successions, e.g. the Llandovery ranges from Ma. Eon PHANEROZOIC CRYPTOZOIC or PRECAMBRIAN Era PALAEOZOIC PROTEROZOIC ARCHAEAN HADEAN Period Permian Carboniferous Devonian Silurian Ordovician Cambrian Neoproterozoic Mesoproterozoic Palaeoproterozoic Late Archaean Middle Archaean Early Archaean Epoch Late Early Silesian Dinantian Late Mid Early Late Early Late Mid Early Late Mid Early Age Zechstein Rotliegendes Stephanian Westphalian Namurian Viséan Tournaisian Famennian Frasnian Givetian Eifelian Emsian Pragian Lochkovian Pridoli Ludlow Wenlock Llandovery Ashgill Caradoc Llanvirn Arenig Tremadoc Ma Figure 1.3 Part of the geological timescale, showing chronostratigraphic subdivisions. Note that formally defined divisions start with an upper case letter (e.g. Mid-Ordovician), whereas informally defined divisions (e.g. mid-silurian) start with a lower case letter. Accordingly, Early Devonian has a specific meaning or definition, whereas early Devonian is less specific.

10 10 Mountain Building in Scotland Disentangling the continents The dating of crystalline rocks using radiogenic isotopes has become a prerequisite to understanding and unravelling regions of complexly deformed and metamorphosed rocks. For several decades, radiogenic isotope systems have been used to date events such as the crystallization of metamorphic and igneous rocks. With the advent of new analytical methods it is now possible to date the crystallization of individual minerals (or even parts of minerals) such as zircon or garnet, to a precision of one or two million years, even in the oldest Precambrian rocks. Our knowledge of continental geology owes much to these methods. For instance, we now know that the succession of collisions or orogenies that have built the present-day continents occurred over long expanses of geological time. Orogenic belts can be made up of several displaced crustal fragments, called terranes, which may have travelled thousands of kilometres across the Earth s surface before colliding with and accreting to an existing continental margin. These terranes can be oceanic crust, island arcs, or pieces of continental crust carried by subducting plates and plastered to continental margins when the plates collided. The collision scar or suture zone may preserve relicts of the oceanic crust that once separated the crustal fragments these relicts are called ophiolites. The rocks that preserve a record of the oldest or most ancient orogenic episodes usually form the core or interior parts of continents these are known as shield areas or cratons. These regions are often surrounded by a series of younger, more recently active mountain belts, which form long, relatively narrow topographic features such as the Alpine Himalayan chain of southern Europe and Asia. As successively younger orogenic belts develop around the margins of the continents, the older orogenic belts that are exposed to these events become incorporated within the younger orogenies, and as a result are progressively reworked. During this process of reworking, the record of the earlier periods of orogeny becomes progressively overprinted by younger events, and so an incomplete record of orogeny is preserved. Several factors may lead to problems in reconstructing the history of ancient orogens. Remnants of older orogens are often obscured and lie beneath younger sedimentary rocks. The older rocks may have complex histories resulting from multiple episodes of deformation, metamorphism and magmatism, which in many cases cannot be resolved even by conventional isotopic methods. The diachronous nature of the successive collisions and accretion of crustal fragments to continental margins during orogeny causes problems of correlation along the belt. In addition, details of early collisions are often obscured by later accretion events. For example, plate boundary histories are difficult to unravel if large-scale strike slip fault systems have been active at different times. 1.4 The collage of ancient orogenic belts in the North Atlantic region The geology of the Scottish Highlands is dominated by the effects of the last great mountain building event to have affected the region the Caledonian Orogeny. However, the Highlands represents only a small fragment of an orogenic belt that was once of much greater extent. Fragments of this early Palaeozoic orogenic belt are scattered across the North Atlantic region as a result

11 Introduction 11 post-caledonian orogens (late Palaeozoic and later) Caledonian Orogen (early mid-palaeozoic) Late Archaean to Proterozoic Archaean cratons main sutures orogen boundaries Caledonian Belt B A L T I C A Tornquist Belt L A U R E N T I A EASTERN AVALONIA ARMORICA Iapetus Suture Appalachian Belt W E S T E R N I A A V A L O N GONDW ANA IBERIA Figure 1.4 Map showing the distribution of ancient continental fragments around Britain and Ireland prior to the opening of the present-day Atlantic Ocean. The age assigned to different continental fragments is that of the most dominant period of orogeny. The younger orogenic belts are built on reworked older orogenic belts. Light shades indicate areas where the geological reconstruction is inferred. of the opening of the present-day Atlantic Ocean. A reconstruction of the position of the continents prior to this opening clearly demonstrates the extent of the Caledonian Orogenic Belt (Figure 1.4). Examination of Figure 1.4 reveals that the Caledonian Orogenic Belt (the Caledonides) has three distinct arms: a northern Caledonian Belt, a western Appalachian Belt and an eastern Tornquist Belt. These belts or branches separate parts of three major palaeocontinents that preserve records of much older orogenic episodes, e.g. the palaeocontinent of Laurentia is composed of rock units that were subjected to major periods of orogeny in both the Archaean and the Proterozoic. The three palaeocontinents of Laurentia (North America and Greenland), Baltica (Scandinavia and the Baltic) and Avalonia (southern Ireland and Britain) drifted together in the early Palaeozoic, colliding to form the Caledonian Orogenic Belt. Britain and Ireland hold a special position in this orogenic system as they straddle the Caledonian Orogen, adjacent to the three palaeocontinents.

12 12 Mountain Building in Scotland 1.5 What caused the Caledonian Orogeny? The tectonics that led to the construction of the Caledonian Orogenic Belt were associated with the closure of a major ocean called Iapetus. The Caledonian Orogeny was not a simple continent continent collision, it encompassed a series of more localized arc arc, arc continent and continent continent collisions. The sequence of events that led to the collision of Laurentia, Baltica and Avalonia, and to the formation of the Caledonian Orogenic Belt, can be traced as far back in time as c. 600 Ma, to the break-up of a major palaeocontinental landmass referred to as the Vendian Supercontinent, named after the Vendian Period (c Ma). This sequence of events is illustrated on Figure 1.5 and can be summarized as follows: The initial break-up of the Vendian Supercontinent began c Ma ago with Baltica rifting from eastern Laurentia along the Greenland margin, and Gondwana rifting from North America, thus forming the Iapetus Ocean (Figures 1.5a,b). The initial stages of ocean destruction began in Cambrian to Early Ordovician times with the formation of subduction zones and the localized collision of volcanic arcs along the margins of the continents that surrounded Iapetus (Figures 1.5c,d). The phase of arc continent collisions along the southern margin of Laurentia is referred to as the Grampian orogenic phase, evidence for which can be seen in the rocks of Scotland and Ireland. Also at this time the continent of Gondwana began to break up, and continental fragments, including Avalonia, which incorporated southern Britain, rifted and migrated northwards, narrowing the intervening Iapetus Ocean and opening another, the Rheic Ocean, in its wake (Figure 1.5d). The initial collision of Avalonian fragments with the Laurentian margin (Figure 1.5e) occurred between c. 470 Ma and c. 440 Ma. The final closure of Iapetus was in the Silurian (c. 425 Ma), with Baltica and parts of Avalonia converging obliquely with the Laurentian margin (Figure 1.5f), resulting in the Scandian orogenic phase. At this time, significant strike slip displacements associated with oblique collision disrupted the Laurentian margin and the Iapetus Suture Zone. 1.6 The tectonic map of Britain and Ireland The Caledonian Orogeny was primarily responsible for the consolidation of the British Isles into its present pattern of fault-bounded crustal blocks. These crustal blocks are terranes that represent displaced fragments of continents, volcanic arcs or ocean basins accreted to the continental margins by combinations of subduction, collision and strike slip displacement. Each of these terranes has its own individual and distinct history. The terranes and major terrane-bounding faults of Britain and Ireland are illustrated in Figure 1.6. These terranes are subdivided into three main groups: Laurentian Terranes: those to the north of the Highland Boundary Fault Fair Head Clew Bay Line, which have evolved as part of Laurentia (Hebridean, Northern Highlands and Central Highlands Terranes). Gondwanan Terranes: those to the south of the Solway Line, which are thought to have evolved as part of Gondwana (Leinster Lakesman, Monian, Welsh Basin and Midland Platform Terranes). Intermediate Accreted Terranes: an intervening zone consisting of slivers of continental margin, island arc and oceanic rocks (Midland Valley and Southern Uplands Terranes) that form a complex suture zone separating Laurentia and the Gondwanan Terranes.

13 Introduction 13 (a) c. 580 Ma Vendian supercontinent SIBERIA (b) Late Neoproterozoic c. 550 Ma SIBERIA 30 S 60 S BALTICA L A U R E N T I A N South Pole S GONDWANA L A U R E N T I A N BALTICA 60 S South Pole S GONDWANA 30 S N Pacific Ocean (c) Early Ordovician c. 490 Ma L A U R E N T I A A r c Tornquist Sea Iapetus Ocean G r a m p i a n SIBERIA S BALTICA South Pole 60 S GONDWANA 30 S Equator N S main regions of rifting and ocean opening major subduction zones positions of northern and southern Britain and Ireland Equator N S Iapetus Ocean (d) Mid-Ordovician c. 470 Ma L A U R E N T I A SIBERIA Tornquist Sea AVALONIA Rheic Ocean BALTICA South Pole 60 S GONDWANA 30 S Equator (e) Early Silurian c. 440 Ma (f) Mid-Silurian c. 425 Ma SIBERIA L A U R E N T I A N S AVALONIA ARMORICA South Pole BALTICA Rheic Ocean Theic Ocean 60 S 30 S Equator 30 N Equator BALTICA 30 S L A U R E N T I A 60 N SIBERIA Rheic Ocean ARMORICA GONDWANA GONDWANA 60 S South Pole Figure 1.5 Global palaeocontinental reconstructions for the late Neoproterozoic and Palaeozoic: (a) c. 580 Ma; (b) c. 550 Ma; (c) c. 490 Ma; (d) c. 470 Ma; (e) c. 440 Ma; (f) c. 425 Ma.

14 14 Mountain Building in Scotland terrane boundaries are delineated according to date of last major displacement 100 km Devonian Ordovician or Silurian Cambrian or earlier Fair Head Clew Bay Line HEBRIDEAN NORTHERN HIGHLANDS Moine Thrust CENTRAL HIGHLANDS (GRAMPIAN) Southern Uplands Fault Great Glen Fault Highland Boundary Fault MIDLAND VALLEY SOUTHERN UPLANDS Solway Line =lapetus Suture Zone LEINSTER LAKESMAN LAURENTIAN TERRANES INTERMEDIATE ACCRETED TERRANES GONDWANAN TERRANES MONIAN WELSH BASIN MIDLAND PLATFORM Variscan Front? LIZARD Figure 1.6 Simplified Palaeozoic terrane map of Britain and Ireland. 1.7 The scope of this book The Scottish Highlands contains some of the most extensively studied areas of geology in the world. Given the fact that the region is of relatively small size, it is perhaps surprising that the rocks of the Scottish Highlands preserve a record of at least six periods of mountain building, which occurred over considerable geological time. In this book we will examine the nature of the evidence and the methods employed by geologists to unravel the complex history of this particular region. As mentioned in Section 1.4, the Caledonian Orogeny was the last major mountain-building event to have left an imprint on this region. In Sections 2 and 3 we will see glimpses of several older orogenic episodes from the Archaean and Proterozoic Eras. These serve to outline the basic concepts and principles of orogenesis, from which a more detailed study of the Caledonian Orogeny can be undertaken. Sections 4 to 9 focus on unravelling what happened during and after the Caledonian Orogeny.

6 Exhumation of the Grampian

6 Exhumation of the Grampian 73 6 Exhumation of the Grampian mountains 6.1 Introduction Section 5 discussed the collision of an island arc with the margin of Laurentia, which led to the formation of a major mountain belt, the Grampian

More information

7 Sedimentation and tectonics at a mid- Ordovician to Silurian active margin

7 Sedimentation and tectonics at a mid- Ordovician to Silurian active margin 80 Mountain Building in Scotland 7 Sedimentation and tectonics at a mid- Ordovician to Silurian active margin 7.1 Introduction In mid-ordovician to Silurian times, the Grampian mountains underwent exhumation,

More information

8 Multiple plate collisions and the end of the Iapetus Ocean

8 Multiple plate collisions and the end of the Iapetus Ocean 86 Mountain Building in Scotland 8 Multiple plate collisions and the end of the Iapetus Ocean 8.1 Introduction Sections 4 to 7 outlined the evidence and possible plate-tectonic explanations for the formation

More information

2 Britain s oldest rocks: remnants of

2 Britain s oldest rocks: remnants of Britain s oldest rocks: remnants of Archaean crust 15 2 Britain s oldest rocks: remnants of Archaean crust 2.1 Introduction Owing to the complex nature of extremely old deformed rocks, the standard methods

More information

Copyright McGraw-Hill Education. All rights reserved. No reproduction or distribution without the prior written consent of McGraw-Hill Education

Copyright McGraw-Hill Education. All rights reserved. No reproduction or distribution without the prior written consent of McGraw-Hill Education Copyright McGraw-Hill Education. All rights reserved. No reproduction or distribution without the prior written consent of McGraw-Hill Education Tibetan Plateau and Himalaya -southern Asia 11.00.a VE 10X

More information

Evolution of Continents Chapter 20

Evolution of Continents Chapter 20 Evolution of Continents Chapter 20 Does not contain complete lecture notes. Mountain belts Orogenesis the processes that collectively produce a mountain belt Includes folding, thrust faulting, metamorphism,

More information

3/5/05 Dr. Stewart 1

3/5/05 Dr. Stewart 1 I. Physiography of Appalachian Mountains A. Introduction 1. These mountains extend from NE Canada to Georgia 2. They are the remains of a deeply eroded, ancient mountain chain once larger than the Himalayans

More information

Geology of the Batemans Bay region. Geological evolution. The Lachlan Orogen

Geology of the Batemans Bay region. Geological evolution. The Lachlan Orogen Australian Journal of Earth Sciences 1 The word orogen is derived from the ancient Greek language word for mountain building. The Lachlan Orogen The rocks exposed in the Batemans Bay are part of the geological

More information

The Building of the NYC Region

The Building of the NYC Region The Building of the NYC Region Definitions Fall Line marks the area where an upland region (continental bedrock) and a coastal plain meet Piedmont the plateau region of the eastern United States which

More information

The Lithosphere and the Tectonic System. The Structure of the Earth. Temperature 3000º ºC. Mantle

The Lithosphere and the Tectonic System. The Structure of the Earth. Temperature 3000º ºC. Mantle The Lithosphere and the Tectonic System Objectives: Understand the structure of the planet Earth Review the geologic timescale as a point of reference for the history of the Earth Examine the major relief

More information

Earth s History. The principle of states that geologic processes that happened in the past can be explained by current geologic processes.

Earth s History. The principle of states that geologic processes that happened in the past can be explained by current geologic processes. Earth s History Date: Been There, Done That What is the principle of uniformitarianism? The principle of states that geologic processes that happened in the past can be explained by current geologic processes.

More information

Section 7. Reading the Geologic History of Your Community. What Do You See? Think About It. Investigate. Learning Outcomes

Section 7. Reading the Geologic History of Your Community. What Do You See? Think About It. Investigate. Learning Outcomes Chapter 3 Minerals, Rocks, and Structures Section 7 Reading the Geologic History of Your Community What Do You See? Learning Outcomes In this section, you will Goals Text Learning Outcomes In this section,

More information

Lithospheric plates. Geology of the Batemans Bay region. Tectonic processes

Lithospheric plates. Geology of the Batemans Bay region. Tectonic processes 1 Lithospheric plates Enormous heat sources in the Earth s deep interior, acquired during the very early history of the planet billions of years ago continue to drive present-day geological at the surface.

More information

Strike-Slip Faults. ! Fault motion is parallel to the strike of the fault.

Strike-Slip Faults. ! Fault motion is parallel to the strike of the fault. Strike-Slip Faults! Fault motion is parallel to the strike of the fault.! Usually vertical, no hanging-wall/footwall blocks.! Classified by the relative sense of motion. " Right lateral opposite block

More information

Mountain Building. Mountain Building

Mountain Building. Mountain Building Mountain Building Mountain building has occurred during the recent geologic past American Cordillera the western margin of the Americas from Cape Horn to Alaska Includes the Andes and Rocky Mountains Alpine

More information

Global Tectonics. Kearey, Philip. Table of Contents ISBN-13: Historical perspective. 2. The interior of the Earth.

Global Tectonics. Kearey, Philip. Table of Contents ISBN-13: Historical perspective. 2. The interior of the Earth. Global Tectonics Kearey, Philip ISBN-13: 9781405107778 Table of Contents Preface. Acknowledgments. 1. Historical perspective. 1.1 Continental drift. 1.2 Sea floor spreading and the birth of plate tectonics.

More information

Chapter 10: Deformation and Mountain Building. Fig. 10.1

Chapter 10: Deformation and Mountain Building. Fig. 10.1 Chapter 10: Deformation and Mountain Building Fig. 10.1 OBJECTIVES Describe the processes of rock deformation and compare and contrast ductile and brittle behavior in rocks. Explain how strike and dip

More information

Continental Landscapes

Continental Landscapes Continental Landscapes Landscape influenced by tectonics, climate & differential weathering Most landforms developed within the last 2 million years System moves toward an equilibrium Continental Landscapes

More information

Chapter 3 Time and Geology

Chapter 3 Time and Geology Chapter 3 Time and Geology Methods of Dating Rocks 1. Relative dating - Using fundamental principles of geology (Steno's Laws, Fossil Succession, etc.) to determine the relative ages of rocks (which rocks

More information

GY 112 Lecture Notes Archean Geology

GY 112 Lecture Notes Archean Geology GY 112 Lecture Notes D. Haywick (2006) 1 GY 112 Lecture Notes Archean Geology Lecture Goals: A) Time frame (the Archean and earlier) B) Rocks and tectonic elements (shield/platform/craton) C) Tectonics

More information

KEY CHAPTER 12 TAKE-HOME QUIZ INTERNAL STRUCTURES AND PROCESSES Score Part B = / 55 PART B

KEY CHAPTER 12 TAKE-HOME QUIZ INTERNAL STRUCTURES AND PROCESSES Score Part B = / 55 PART B GEOLOGY 12 KEY CHAPTER 12 TAKE-HOME QUIZ INTERNAL STRUCTURES AND PROCESSES Score Part B = / 55 PART B CHAPTER 12 Isostacy and Structural Geology 1. Using the terms below, label the following diagrams and

More information

In the space provided, write the letter of the definition that best matches the term or phrase.

In the space provided, write the letter of the definition that best matches the term or phrase. Skills Worksheet Directed Reading Section: The Changing Continents 1. What is the result of slow movements of tectonic plates? RESHAPING EARTH S CRUST In the space provided, write the letter of the definition

More information

Deformation of Rocks. Orientation of Deformed Rocks

Deformation of Rocks. Orientation of Deformed Rocks Deformation of Rocks Folds and faults are geologic structures caused by deformation. Structural geology is the study of the deformation of rocks and its effects. Fig. 7.1 Orientation of Deformed Rocks

More information

Chapter 10: Volcanoes and Other Igneous Activity Section 1: The Nature of Volcanic Eruptions I. Factors Affecting Eruptions Group # Main Idea:

Chapter 10: Volcanoes and Other Igneous Activity Section 1: The Nature of Volcanic Eruptions I. Factors Affecting Eruptions Group # Main Idea: Chapter 10: Volcanoes and Other Igneous Activity Section 1: The Nature of Volcanic Eruptions I. Factors Affecting Eruptions Group # A. Viscosity Group # B. Dissolved Gases Group # II. Volcanic Material

More information

GO ON. Directions: Use the diagram below to answer question 1.

GO ON. Directions: Use the diagram below to answer question 1. d i a g n o s t i c t e s t : e a r t h a n d s p a c e s c i e n c e question 1. 1. What is the correct order (starting from the surface) of Earth s layers? A crust, outer core, inner core, mantle B mantle,

More information

Work Package 3. Drifting Apart Story

Work Package 3. Drifting Apart Story Work Package 3 Drifting Apart Story Contents 1 Drifting Apart 2 Our dynamic planet 3 Plate tectonic theory a. Continental drift b. Sea-floor spreading c. Wilson cycles 4 Drifting Apart storyline a. Ancient

More information

Section 10.1 The Nature of Volcanic Eruptions This section discusses volcanic eruptions, types of volcanoes, and other volcanic landforms.

Section 10.1 The Nature of Volcanic Eruptions This section discusses volcanic eruptions, types of volcanoes, and other volcanic landforms. Chapter 10 Section 10.1 The Nature of Volcanic Eruptions This section discusses volcanic eruptions, types of volcanoes, and other volcanic landforms. Reading Strategy Previewing Before you read the section,

More information

GLY 155 Introduction to Physical Geology, W. Altermann. Press & Siever, compressive forces. Compressive forces cause folding and faulting.

GLY 155 Introduction to Physical Geology, W. Altermann. Press & Siever, compressive forces. Compressive forces cause folding and faulting. Press & Siever, 1995 compressive forces Compressive forces cause folding and faulting. faults 1 Uplift is followed by erosion, which creates new horizontal surface. lava flows Volcanic eruptions cover

More information

History of Earth. Chapter 9: HISTORY OF EARTH. The Solar System. Early Earth: A Giant Impact! Early Earth. Formation of the Solar System

History of Earth. Chapter 9: HISTORY OF EARTH. The Solar System. Early Earth: A Giant Impact! Early Earth. Formation of the Solar System Chapter 9: HISTORY OF EARTH The Essential Earth, 2 nd Edition Thomas H. Jordan & John Grotzinger History of Earth Earth is 4.56 Billion Years Old Earth has experienced a rich and diverse history that we

More information

Deep Time: How Old Is Old?

Deep Time: How Old Is Old? Deep Time: How Old Is Old? Updated by: Rick Oches, Professor of Geology & Environmental Sciences Bentley University Waltham, Massachusetts Based on slides prepared by: Ronald L. Parker, Senior Geologist

More information

Name Class Date. In the space provided, write the letter of the definition that best matches the term or phrase.

Name Class Date. In the space provided, write the letter of the definition that best matches the term or phrase. Skills Worksheet Directed Reading Section: The Changing Continents 1. What is the result of slow movements of tectonic plates? RESHAPING EARTH S CRUST In the space provided, write the letter of the definition

More information

Deep Time: How Old Is Old?

Deep Time: How Old Is Old? Deep Time: How Old Is Old? Updated by: Based on slides prepared by: Rick Oches, Professor of Geology & Environmental Sciences Bentley University Waltham, Massachusetts Ronald L. Parker, Senior Geologist

More information

State the principle of uniformitarianism. Explain how the law of superposition can be used to determine the relative age of rocks.

State the principle of uniformitarianism. Explain how the law of superposition can be used to determine the relative age of rocks. Objectives State the principle of uniformitarianism. Explain how the law of superposition can be used to determine the relative age of rocks. Compare three types of unconformities. Apply the law of crosscutting

More information

Chapter 10. Early Paleozoic Events

Chapter 10. Early Paleozoic Events Chapter 10 Early Paleozoic Events The Phanerozoic Eon Consists of three eras (from oldest to youngest): Paleozoic = "ancient life" (542-251 m.y. ago) Mesozoic = "middle life" (251-65.5 m.y. ago) Cenozoic

More information

Plate Tectonics. entirely rock both and rock

Plate Tectonics. entirely rock both and rock Plate Tectonics I. Tectonics A. Tectonic Forces are forces generated from within Earth causing rock to become. B. 1. The study of the origin and arrangement of Earth surface including mountain belts, continents,

More information

Beneath our Feet: The 4 Layers of the Earty by Kelly Hashway

Beneath our Feet: The 4 Layers of the Earty by Kelly Hashway Beneath our Feet: The 4 Layers of the Earty by Kelly Hashway The Earth is more than a giant ball made up of dirt, rocks, and minerals. The Earth may look like a giant ball from when looking at it from

More information

Lecture #13 notes, Geology 3950 Spring 2006: CR Stern Magnetic reversals (text pages th edition and in the 5 th edition)

Lecture #13 notes, Geology 3950 Spring 2006: CR Stern Magnetic reversals (text pages th edition and in the 5 th edition) Lecture #13 notes, Geology 3950 Spring 2006: CR Stern Magnetic reversals (text pages 35-37 4 th edition and 53-55 in the 5 th edition) The earth has a magnetic field generated by circulation of charged

More information

Geologic History. Earth is very, very old

Geologic History. Earth is very, very old Geologic History Earth is very, very old Earth s History The history of Earth and the ages of rocks can be investigated and understood by studying rocks and fossils. Evidence of ancient, often extinct

More information

NAME HOMEWORK ASSIGNMENT #4 MATERIAL COVERS CHAPTERS 19, 20, 21, & 2

NAME HOMEWORK ASSIGNMENT #4 MATERIAL COVERS CHAPTERS 19, 20, 21, & 2 NAME HOMEWORK ASSIGNMENT #4 MATERIAL COVERS CHAPTERS 19, 20, 21, & 2 Assignment is due the beginning of the class period on December 14, 2004. Mark answers on a scantron sheet, which will be provided.

More information

Section 1: Continental Drift

Section 1: Continental Drift Plate Tectonics Section 1 Section 1: Continental Drift Preview Key Ideas Wegener s Hypothesis Sea-Floor Spreading Paleomagnetism Wegener Redeemed Continental Drift (Pangaea) Plate Tectonics Section 1 Key

More information

Geologic Structures. Changes in the shape and/or orientation of rocks in response to applied stress

Geologic Structures. Changes in the shape and/or orientation of rocks in response to applied stress Geologic Structures Changes in the shape and/or orientation of rocks in response to applied stress Figure 15.19 Can be as big as a breadbox Or much bigger than a breadbox Three basic types Fractures >>>

More information

Earth Science. Name Block. Unit 3 Review Worksheet. Circle the letter that corresponds to the correct answer

Earth Science. Name Block. Unit 3 Review Worksheet. Circle the letter that corresponds to the correct answer Earth Science Unit 3 Review Worksheet Name Block Circle the letter that corresponds to the correct answer 1. Which geologic principle is used when a geologist observes an outcrop or rocks and determines

More information

NC Earth Science Essential Standards

NC Earth Science Essential Standards NC Earth Science Essential Standards EEn. 2.1 Explain how processes and forces affect the Lithosphere. EEn. 2.1.1 Explain how the rock cycle, plate tectonics, volcanoes, and earthquakes impact the Lithosphere.

More information

Unit 6: Interpreting Earth s History

Unit 6: Interpreting Earth s History Unit 6: Interpreting Earth s History How do we know that the Earth has changed over time? Regent s Earth Science Name: Topics Relative Dating Uniformitarianism Superposition Original Horizontality Igneous

More information

Prentice Hall EARTH SCIENCE

Prentice Hall EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 12 Geologic Time 12.1 Discovering Earth s History Rocks Record Earth History Rocks record geological events and changing life forms of the past. We have

More information

geologic age of Earth - about 4.6 billion years

geologic age of Earth - about 4.6 billion years Geologic Time Geologic Time geologic age of Earth - about 4.6 billion years Geologic Time very difficult to appreciate from our human perspective necessary to understand history of Earth two basic ways

More information

Plate Tectonics 22/12/2017

Plate Tectonics 22/12/2017 Map of the tectonic plates. Plate Tectonics In 1912 the meteorologist Alfred Wegener independently developed what he called continental drift, (expanded in his 1915 book The Origin of Continents and Oceans).

More information

Lecture Outlines PowerPoint. Chapter 10 Earth Science, 12e Tarbuck/Lutgens

Lecture Outlines PowerPoint. Chapter 10 Earth Science, 12e Tarbuck/Lutgens Lecture Outlines PowerPoint Chapter 10 Earth Science, 12e Tarbuck/Lutgens 2009 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors

More information

3. The diagram below shows how scientists think some of Earth's continents were joined together in the geologic past.

3. The diagram below shows how scientists think some of Earth's continents were joined together in the geologic past. 1. The map below shows the present-day locations of South America and Africa. Remains of Mesosaurus, an extinct freshwater reptile, have been found in similarly aged bedrock formed from lake sediments

More information

A) B) C) D) 4. Which diagram below best represents the pattern of magnetic orientation in the seafloor on the west (left) side of the ocean ridge?

A) B) C) D) 4. Which diagram below best represents the pattern of magnetic orientation in the seafloor on the west (left) side of the ocean ridge? 1. Crustal formation, which may cause the widening of an ocean, is most likely occurring at the boundary between the A) African Plate and the Eurasian Plate B) Pacific Plate and the Philippine Plate C)

More information

Lecture Outline Friday Feb. 21 Wednesday Feb. 28, 2018

Lecture Outline Friday Feb. 21 Wednesday Feb. 28, 2018 Lecture Outline Friday Feb. 21 Wednesday Feb. 28, 2018 Questions? Key Points for today What are the 5 relative age dating principles and how do you apply the principles to determine a geologic history

More information

Rock cycle diagram. Principle of Original Horizontality. Sediment is deposited horizontally

Rock cycle diagram. Principle of Original Horizontality. Sediment is deposited horizontally Geologic Time Rock cycle diagram Leaves of History Chapter 21 Lateral Continuity Principle of Original Horizontality Sediment is deposited horizontally Principle of Superposition Oldest rock A Younger

More information

Refer to the map on page 173 to answer the following questions.

Refer to the map on page 173 to answer the following questions. Chapter 8-1 Plate Tectonics 1. Brainstorm the type of evidence that would indicate a climate change and how this evidence supports the theory of continental drift. Tropical fossils in cold regions Evidence

More information

Do Now: Vocabulary: Objectives. Vocabulary: 1/5/2016. Wegener? (Can they move?) the idea that continents have moved over time?

Do Now: Vocabulary: Objectives. Vocabulary: 1/5/2016. Wegener? (Can they move?) the idea that continents have moved over time? Do Now: 1. Who was Alfred Wegener? 2. What was Pangaea? 3. Are continents fixed? (Can they move?) 4. What evidence supports the idea that continents have moved over time? Objectives What evidence suggests

More information

6. In the diagram below, letters A and B represent locations near the edge of a continent.

6. In the diagram below, letters A and B represent locations near the edge of a continent. 1. Base your answer to the following question on the cross section below and on your knowledge of Earth science. The cross section represents the distance and age of ocean-floor bedrock found on both sides

More information

The Building of a Continent. Delving into Deep Time

The Building of a Continent. Delving into Deep Time The Building of a Continent Delving into Deep Time Methods for Studying the Past Identifying orogenies Mountain building events Mountains erode Can t study topography Study the evidence they leave behind

More information

Captain s Tryouts 2017

Captain s Tryouts 2017 Captain s Tryouts 2017 Dynamic Planet Test Written by: Araneesh Pratap (Chattahoochee High School) Name: Date: Answer all questions on the answer sheet. Point values are given next to each question or

More information

Geosphere Final Exam Study Guide

Geosphere Final Exam Study Guide Geosphere Final Exam Study Guide Chapter 1 Intro to Earth Systems 1. Name and describe Earth s 4 major spheres Geosphere-- nonliving, mostly solid rock divided into crust, mantle, and core Atmosphere a

More information

Mesozoic Earth History

Mesozoic Earth History Mesozoic Earth History The Mesozoic Era 251-66 MYA Breakup of Pangea Changes in air and oceanic currents Evolution of new terrestrial and marine life Opening of the Atlantic Ocean Basin Rocky Mountains

More information

The Earth s Structure. The Lithosphere and Tectonic. The Lithosphere and Tectonic. System. Chapter 12. The Earth s Interior

The Earth s Structure. The Lithosphere and Tectonic. The Lithosphere and Tectonic. System. Chapter 12. The Earth s Interior The Lithosphere and Tectonic System Chapter 12 The Lithosphere and Tectonic System The theory describing the changing configuration of the continents through time is called plate tectonics. Plate tectonic

More information

Questions and Topics

Questions and Topics Plate Tectonics and Continental Drift Questions and Topics 1. What are the theories of Plate Tectonics and Continental Drift? 2. What is the evidence that Continents move? 3. What are the forces that

More information

Plate Tectonics Practice Test

Plate Tectonics Practice Test Plate Tectonics Practice Test 1. What is the main idea Alfred Wegner proposed in the Theory of Continental Drift that he published in 1915? a. The continents float on a liquid layer that allows them to

More information

Geologic Trips San Francisco and the Bay Area

Geologic Trips San Francisco and the Bay Area Excerpt from Geologic Trips San Francisco and the Bay Area by Ted Konigsmark ISBN 0-9661316-4-9 GeoPress All rights reserved. No part of this book may be reproduced without written permission in writing,

More information

PHYSICAL GEOLOGY AND THE ENVIRONMENT (2 ND CANADIAN EDITION)

PHYSICAL GEOLOGY AND THE ENVIRONMENT (2 ND CANADIAN EDITION) Chapter 2: Plate Tectonics Chapter Summary: Plate tectonics is a theory that suggests Earth's surface is divided into several large plates that change position and size. Intense geologic activity occurs

More information

Earth Science Lesson Plan Quarter 3, Week 7, Day 1

Earth Science Lesson Plan Quarter 3, Week 7, Day 1 Earth Science Lesson Plan Quarter 3, Week 7, Day 1 Outcomes for Today Standard Focus: PREPARE 1. Background knowledge necessary for today s reading. Continental ice sheets increase the weight of the Earth

More information

Earth s Dynamic Surface

Earth s Dynamic Surface Earth s Dynamic Surface Shaping Earth s Surface What do you think? Read the two statements below and decide whether you agree or disagree with them. Place an A in the Before column if you agree with the

More information

11.1 Rock Deformation

11.1 Rock Deformation Tarbuck Lutgens Mountain Building 11.1 Rock Deformation Factors Affecting Deformation Factors that influence the strength of a rock and how it will deform include temperature, confining pressure, rock

More information

Terrain Units PALEOGEOGRAPHY: LANDFORM CREATION. Present Geology of NYS. Detailed Geologic Map of NYS

Terrain Units PALEOGEOGRAPHY: LANDFORM CREATION. Present Geology of NYS. Detailed Geologic Map of NYS NYS TOPOGRAPHY Why so? PALEOGEOGRAPHY: LANDFORM CREATION Prof. Anthony Grande AFG 014 Present Geology of NYS Detailed Geologic Map of NYS Generalized Geology Detailed Geology Hot links to the fold out

More information

Plate Tectonics GEOL 101 Lecture 22 How Are Mountains Built?

Plate Tectonics GEOL 101 Lecture 22 How Are Mountains Built? Plate Tectonics GEOL 101 Lecture 22 How Are Mountains Built? The Grand Tetons, Wyoming First a Brief Review of Sea Floor Spreading Prop: Test 3 Invitations Break-Up of a Continent and Origin of an Ocean

More information

Plate Tectonic Vocabulary Chapter 10 Pages

Plate Tectonic Vocabulary Chapter 10 Pages Name: Period: Plate Tectonic Vocabulary Chapter 10 Pages 239-260 Vocabulary Word What is this? What are some examples? What does it look like? (draw a picture or diagram) Continental drift Mid-ocean ridge

More information

Chapter. Mountain Building

Chapter. Mountain Building Chapter Mountain Building 11.1 Rock Deformation Factors Affecting Deformation Factors that influence the strength of a rock and how it will deform include temperature, confining pressure, rock type, and

More information

2011 Pearson Education, Inc. 1

2011 Pearson Education, Inc. 1 1 An Introduction to Geology Earth, 10e - Chapter 1 Stan Hatfield Southwestern Illinois College 3 The Science of Geology Geology is the science that pursues an understanding of planet Earth. Physical geology

More information

Section 1: How Did Life Begin? Chapter 19: History of Life on Earth. Section 2: The Age of Earth

Section 1: How Did Life Begin? Chapter 19: History of Life on Earth. Section 2: The Age of Earth Chapter 19: History of Life on Earth Section 1: How Did Life Begin? I. The Basic Chemicals of Life A. 1920s B. Earth s early oceans contained large amounts of organic molecules C. Molecules formed spontaneously

More information

Composition of the earth, Geologic Time, and Plate Tectonics

Composition of the earth, Geologic Time, and Plate Tectonics Composition of the earth, Geologic Time, and Plate Tectonics Layers of the earth Chemical vs. Mechanical Chemical : Mechanical: 1) Core: Ni and Fe 2) Mantle: Mostly Peridotite 3) Crust: Many different

More information

REGIONAL PERSPECTIVES

REGIONAL PERSPECTIVES 2917-CH20.pdf 11/20/03 5:24 PM Page 501 PART E REGIONAL PERSPECTIVES 501 2917-CH20.pdf 11/20/03 5:24 PM Page 502 C H A P T E R T W E N T Y A Global View 20.1 Introduction 502 20.2 Global Deformation Patterns

More information

Ordovician. System. Cambrian. System

Ordovician. System. Cambrian. System 443 495 543 Late Middle Early Late Middle Early Ordovician System Cambrian System Earth History, Ch. 13 1 Ch. 13 Review: Early Paleozoic life & Burgess Shale fauna Most animal phyla originated in Cambrian;

More information

Plate Tectonics: A Unifying Theory

Plate Tectonics: A Unifying Theory Plate Tectonics: A Unifying Theory What is Plate Tectonics? - 7 large tectonic plates and many smaller ones that break up the lithosphere - Plates are brittle and float on asthenosphere and glide past

More information

Tectonic plates of the world

Tectonic plates of the world Mountain Building Tectonic plates of the world ISOSTACY Isostatic Rebound crust rises as a result of removal of mass This iceberg also demonstrates the process of isostatic rebound. Types of Mountains

More information

The continental lithosphere

The continental lithosphere Simplicity to complexity: The continental lithosphere Reading: Fowler p350-377 Sampling techniques Seismic refraction Bulk crustal properties, thickness velocity profiles Seismic reflection To image specific

More information

Prentice Hall EARTH SCIENCE

Prentice Hall EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 9 Plate Tectonics 9.1 Continental Drift An Idea Before Its Time Wegener s continental drift hypothesis stated that the continents had once been joined

More information

Prentice Hall EARTH SCIENCE

Prentice Hall EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 9 Plate Tectonics 9.1 Continental Drift An Idea Before Its Time Wegener s continental drift hypothesis stated that the continents had once been joined

More information

Do NOT open the test until instructed to do so.

Do NOT open the test until instructed to do so. Raw Score: Rank: School: Team Number: Names: Boyceville Invitational, December 2, 2017 Dynamic Planet Plate Tectonics and Geographical Impacts Do NOT open the test until instructed to do so. 2011 Tohoku

More information

Earth Science, (Tarbuck/Lutgens) Chapter 10: Mountain Building

Earth Science, (Tarbuck/Lutgens) Chapter 10: Mountain Building Earth Science, (Tarbuck/Lutgens) Chapter 10: Mountain Building 1) A(n) fault has little or no vertical movements of the two blocks. A) stick slip B) oblique slip C) strike slip D) dip slip 2) In a(n) fault,

More information

Age of Earth/Geologic Time. Vocabulary

Age of Earth/Geologic Time. Vocabulary Age of Earth/Geologic Time Vocabulary Big Ideas Geologic Time Earth Structures Identify current methods for measuring the age of Earth and its parts, including the law of superposition and radioactive

More information

Continental Drift and Plate Tectonics

Continental Drift and Plate Tectonics Continental Drift and Plate Tectonics Continental Drift Wegener s continental drift hypothesis stated that the continents had once been joined to form a single supercontinent. Wegener proposed that the

More information

Earth History 870:035

Earth History 870:035 Earth History 870:035 Course goal: To describe the history of Earth and its inhabitants Most of Earth s history predates humanity, so it has not been observed Therefore, we will emphasize how scientists

More information

2011 Pearson Education, Inc. 1

2011 Pearson Education, Inc. 1 1 Earth: An Introduction to Physical Geology, 10e Tarbuck & Lutgens An Introduction to Geology Earth, 10e - Chapter 1 Stan Hatfield Southwestern Illinois College 4 The Science of Geology Geology is the

More information

Forces That Shape Earth. How do continents move? What forces can change rocks? How does plate motion affect the rock cycle?

Forces That Shape Earth. How do continents move? What forces can change rocks? How does plate motion affect the rock cycle? Forces That Shape Earth How do continents move? What forces can change rocks? How does plate motion affect the rock cycle? Plate Motion Mountain ranges are produced by plate tectonics. The theory of plate

More information

Earth overall average density = 5.5 g/cm 3 Temp increases with depth, the thermal gradient 30 0 C/km Pressure and the density also increase with

Earth overall average density = 5.5 g/cm 3 Temp increases with depth, the thermal gradient 30 0 C/km Pressure and the density also increase with Plate Tectonics Earth Earth overall average density = 5.5 g/cm 3 Temp increases with depth, the thermal gradient 30 0 C/km Pressure and the density also increase with depth Spheroid: with a longer major

More information

GEOLOGICAL TIME / DATING TECHNIQUES

GEOLOGICAL TIME / DATING TECHNIQUES DATE DUE: INSTRUCTOR: TERRY J. BOROUGHS Geology 305 NAME: SECTION: GEOLOGICAL TIME / DATING TECHNIQUES Instructions: Read each question carefully before selecting the BEST answer. Provide specific and

More information

Plate Tectonics. Chapter 17. Great Idea: The entire Earth is still changing, due to the slow convection of soft, hot rocks deep within the planet.

Plate Tectonics. Chapter 17. Great Idea: The entire Earth is still changing, due to the slow convection of soft, hot rocks deep within the planet. Plate Tectonics Chapter 17 Great Idea: The entire Earth is still changing, due to the slow convection of soft, hot rocks deep within the planet. 1 Chapter Outline The Dynamic Earth Plate Tectonics: A Unifying

More information

Name: Date: Period: Page 1

Name: Date: Period: Page 1 Name: Date: Period: Base your answers to questions 1 through 4 on the three bedrock outcrops below and on your knowledge of Earth science. The outcrops, labeled I, II, and III, are located within 15 kilometers

More information

Directed Reading page

Directed Reading page Skills Worksheet Directed Reading page 185-190 Section: Determining Relative Age 1. How old is Earth estimated to be? 2. Who originated the idea that Earth is billions of years old? 3. On what did the

More information

Continental drift

Continental drift Plate Tectonics Continental drift Continental drift Continental drift Continental drift Continental drift Plate Tectonics Plate Tectonics Continental Drift and Paleomagnetism Paleomagnetism Renewed interest

More information

Directed Reading. Section: How Mountains Form MOUNTAIN RANGES AND SYSTEMS. Skills Worksheet

Directed Reading. Section: How Mountains Form MOUNTAIN RANGES AND SYSTEMS. Skills Worksheet Skills Worksheet Directed Reading Section: How Mountains Form 1. How high is Mount Everest? a. about 1980 km above sea level b. more than 8 km below sea level c. more than 8 km above sea level d. more

More information

Lecture 2: Basin evolution in NW Europe in the Carboniferous: past legacies and plate tectonics. Links to North American geology and global controls

Lecture 2: Basin evolution in NW Europe in the Carboniferous: past legacies and plate tectonics. Links to North American geology and global controls Lecture 2: Basin evolution in NW Europe in the Carboniferous: past legacies and plate tectonics. Links to North American geology and global controls on sedimentation. Aims Examine broad global setting

More information

(1) Identify 5 major principles of relative dating? For each principle, describe how you tell what is younger and what is older.

(1) Identify 5 major principles of relative dating? For each principle, describe how you tell what is younger and what is older. Things to Know - Third GLG101Exam Page 1 Important Note: This is not everything you need to know or study. However, it provides you with a relatively comprehensive list of questions to help you study.

More information

Dynamic Crust Practice

Dynamic Crust Practice 1. Base your answer to the following question on the cross section below and on your knowledge of Earth science. The cross section represents the distance and age of ocean-floor bedrock found on both sides

More information

ENVI.2030L Geologic Time

ENVI.2030L Geologic Time Name ENVI.2030L Geologic Time I. Introduction There are two types of geologic time, relative and absolute. In the case of relative time geologic events are arranged in their order of occurrence. No attempt

More information

Plate Tectonics - Demonstration

Plate Tectonics - Demonstration Name: Reference: Prof. Larry Braile - Educational Resources Copyright 2000. L. Braile. Permission granted for reproduction for non-commercial uses. http://web.ics.purdue.edu/~braile/indexlinks/educ.htm

More information